Astrophysics

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89 Terms

1
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mass

the amount of substance or matter that an object contains

<p>the amount of substance or matter that an object contains</p>
2
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weight

the force of gravity pulling the mass of the object

<p>the force of gravity pulling the mass of the object</p>
3
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formula for weight

weight, W (in N) = Mass, m (in kg) * Gravitational Field Strength, g (in N/kg)

<p>weight, W (in N) = Mass, m (in kg) * Gravitational Field Strength, g (in N/kg)</p>
4
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what factors may affect the gravitational field strength?

most significant - the larger the mass of a planet the greater the gravitational field strength

least significant - the larger the radius of a planet the smaller the gravitational field strength at its surface

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planets in order from the sun

Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune

6
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what makes the planets travel in a circular path?

gravitational forces make the planets follow curved paths; a pulling force has to be applied to make the ball travel in a circle

7
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the size of the gravitational force depends on the:

masses of the 2 objects -> the greater the masses of the 2 objects the stronger the attractive forces between them

distance between the masses - if the distance between the masses is increased the forces between them decrease

<p>masses of the 2 objects -> the greater the masses of the 2 objects the stronger the attractive forces between them</p><p>distance between the masses - if the distance between the masses is increased the forces between them decrease</p>
8
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relationship between mass and force formula

m ɑ F, 2m ɑ 2F, 3m ɑ 3F

9
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relationship between distance and force formula

d ɑ 1/F^2, 2d ɑ 1/(2F)^2, 3d ɑ 1/(3F)^2

10
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formula for speed

speed, v (m/s) = distance, s (m)/time, t (s)

<p>speed, v (m/s) = distance, s (m)/time, t (s)</p>
11
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formula for orbital speed

orbital speed, v (m/s) = circumference of a circle, 2πr (m)/time period, T (s)

<p>orbital speed, v (m/s) = circumference of a circle, 2πr (m)/time period, T (s)</p>
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time/orbital period

the time taken for an object to complete 1 orbit

13
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what type of quantity is weight?

vector

14
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what type of quantity is mass?

scalar

15
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the ... of an object never changes

the ... of an object changes by the gravitational field strength in different places

mass, weight

16
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asteroid

a lump of solid rock and metal that orbit the sun

<p>a lump of solid rock and metal that orbit the sun</p>
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meteorite

when a meteoroid survives a trip through the atmosphere and hits the ground

<p>when a meteoroid survives a trip through the atmosphere and hits the ground</p>
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meteor

when meteoroids enter Earth's atmosphere (or that of another planet, like Mars)

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meteoroid

objects in space that range in size from dust grains to small asteroids

<p>objects in space that range in size from dust grains to small asteroids</p>
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shooting star

a small, rapidly moving meteor burning up on entering the earth's atmosphere

<p>a small, rapidly moving meteor burning up on entering the earth's atmosphere</p>
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comets

balls of dust, rocks and frozen gas

<p>balls of dust, rocks and frozen gas</p>
22
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describe the orbit of a comet

highly elliptical

<p>highly elliptical</p>
23
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describe the speed of a comet throughout its orbit

fastest closest to the sun & slowest furthest from the sun as strongest gravitational force closes t to the sun & weakest gravitational force furthest from the sun

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galaxy

the cluster of billions of stars that all orbit the same point

<p>the cluster of billions of stars that all orbit the same point</p>
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the milky way galaxy

the name of our galaxy, a spiral galaxy that contains about 200-400 billion stars

<p>the name of our galaxy, a spiral galaxy that contains about 200-400 billion stars</p>
26
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what do planets orbit?

sun

<p>sun</p>
27
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what does the moon orbit?

planet

<p>planet</p>
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what do comets orbit?

sun

<p>sun</p>
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what do asteroids orbit?

sun

<p>sun</p>
30
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what do artificial satellites orbit?

any object/body in solar system

<p>any object/body in solar system</p>
31
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stellar evolution of solar mass stars

stellar nebula -> protostar -> main sequence star -> red giant -> white dwarf -> black dwarf

<p>stellar nebula -> protostar -> main sequence star -> red giant -> white dwarf -> black dwarf</p>
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what is a nebula?

cloud of dust and hydrogen gas

<p>cloud of dust and hydrogen gas</p>
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what happens in the nebula stage?

1) Cloud of dust & hydrogen gas

2) Gravity pulls it together

3) Core gets denser

4) GPE is changed into thermal energy

5) Temperature and pressure increases

<p>1) Cloud of dust & hydrogen gas</p><p>2) Gravity pulls it together</p><p>3) Core gets denser</p><p>4) GPE is changed into thermal energy</p><p>5) Temperature and pressure increases</p>
34
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what happens in the protostar stage?

1) More mass is pulled together

2) Core gets even denser

3) Temperature and pressure further increases

4) Nuclear fusion starts - hydrogen fusion

5) Star begins to glow

<p>1) More mass is pulled together</p><p>2) Core gets even denser</p><p>3) Temperature and pressure further increases</p><p>4) Nuclear fusion starts - hydrogen fusion</p><p>5) Star begins to glow</p>
35
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what happens in the main sequence star stage?

1) Nuclear fusion - hydrogen nuclei fuse together to make helium nuclei

2) Outward energy pressure from heat is balanced with inward pull of gravity

3) Long stable period

<p>1) Nuclear fusion - hydrogen nuclei fuse together to make helium nuclei</p><p>2) Outward energy pressure from heat is balanced with inward pull of gravity</p><p>3) Long stable period</p>
36
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what happens in the red giant stage?

1) Hydrogen runs out

2) Core collapses due to unbalance between energy pressure and gravity

3) Core temperature rises again

4) Helium fusion starts

5) Outer layers swell up

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what happens in the white dwarf stage?

1) Fusion slowly stops

2) Star ejects outer layer of dust and gas as a planetary nebula

3) Core collapses due to gravity

<p>1) Fusion slowly stops</p><p>2) Star ejects outer layer of dust and gas as a planetary nebula</p><p>3) Core collapses due to gravity</p>
38
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what happens in the black dwarf stage?

1) Hot dense core left behind

2) No fusion

3) Star cools and fades away

4) Turns into black dwarf

<p>1) Hot dense core left behind</p><p>2) No fusion</p><p>3) Star cools and fades away</p><p>4) Turns into black dwarf</p>
39
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what happens in the red super giant stage?

1) Hydrogen runs out

2) Core collapses due to unbalance between pressure and gravity

3) Outer layers swell up and cool

4) Helium fusion starts

<p>1) Hydrogen runs out</p><p>2) Core collapses due to unbalance between pressure and gravity</p><p>3) Outer layers swell up and cool</p><p>4) Helium fusion starts</p>
40
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what happens in the supernova stage?

1) Expands and contracts several times

2) Heavier elements form

3) Star explodes

4) Ejects outer layer of dust and gas into space

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what happens in the black hole stage?

1) If the core massive enough x4 of our sun

2) Gravity collapses it into a black hole

3) No wave or matter escapes from its gravity

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elements in red super giant from outermost to innermost

hydrogen -> helium -> carbon, oxygen -> Si, S -> iron

43
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colour of stars relative to surface temperature

-a v. hot star emits more blue in its spectrum and therefore looks blue

-a medium star like our Sun looks yellow

-cooler stars appear red

44
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what are the different classes of stars from hottest to coolest

Oh, Be, A, Fine, Girl/guy, Kiss, Me

45
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astronomical objects cool as they ... and heat up as they ...

expand, contract

46
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the brightness of a star depends on

1. the distance the star is from earth

2. what the star is made from and the kinds of nuclear reactions that are taking place / how much light the star emits

<p>1. the distance the star is from earth</p><p>2. what the star is made from and the kinds of nuclear reactions that are taking place / how much light the star emits</p>
47
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what are the 3 different ways in which astronomers describe the brightness of a star

-the apparent brightness/magnitude of a star

-the absolute brightness/magnitude

-the luminosity of a star

48
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the luminosity of a star

a measure of how much energy in the form of light is emitted from a star's surface every second

49
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the absolute brightness/magnitude

a measure of how bright stars would appear if they were placed at the same distance away from the Earth (standard distance = 10 parsecs or 32.6 light years or 3.04*10^14 km)

50
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the apparent brightness/magnitude of a star

a measure of how bright a star is seen from earth

<p>a measure of how bright a star is seen from earth</p>
51
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absolute magnitude scale

runs back to front:

-the brighter the star, the smaller the magnitude

-the dimmer the star, the larger the magnitude

<p>runs back to front:</p><p>-the brighter the star, the smaller the magnitude</p><p>-the dimmer the star, the larger the magnitude</p>
52
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the hertzsprung-russel diagram

relationship between the brightness, and temperature of a star

<p>relationship between the brightness, and temperature of a star</p>
53
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spectrometry

splitting the light into its spectrum

54
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spectrometer

a device that contains something that can split up the different wavelengths

<p>a device that contains something that can split up the different wavelengths</p>
55
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heated filament or candle produces a ... emission spectrum

continuous

<p>continuous</p>
56
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heated element/gases e.g heated hydrogen gas produce a ... emission spectrum

line

<p>line</p>
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if you observe the heated filament or candle through a cool element/gas you see a ... ... spectrum

line absorption

<p>line absorption</p>
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what are the dark bands?

absorption lines and are missing wavelengths (frequencies)

59
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red shift

-the dark bands are absorption lines and are missing wavelengths

-the dark bands are shifted

-the dark bands are shifted to the red end of the spectrum

-the red end of the spectrum is the low frequency, long wavelength end

60
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the doppler effect

the apparent change in the frequency of a sound caused by the motion of either the listener or the source of the sound

<p>the apparent change in the frequency of a sound caused by the motion of either the listener or the source of the sound</p>
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what does the red shift mean in terms of movement?

-if the dark bands are shifted to the red end of the spectrum

-which is the low frequency, long wavelength end of the spectrum

-those stars in the galaxy must be moving away from earth

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the doppler equation

change in wavelength/reference wavelength = velocity of galaxy, v/speed of light, c

63
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big bang theory

universe started 13.5 billion years ago from a single point of high density and pressure

<p>universe started 13.5 billion years ago from a single point of high density and pressure</p>
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what is the evidence of the bing bang theory?

red shift & CMBR

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what is an orbit?

curved path of one celestial object/spacecraft around another celestial object

<p>curved path of one celestial object/spacecraft around another celestial object</p>
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how long does a main sequence star last?

until all of the hydrogen is used up which could be millions/billions of years

<p>until all of the hydrogen is used up which could be millions/billions of years</p>
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what 2 things could form after a supernova? what determines which is formed?

if the star was large, it would condense to a neutron star

if the star was very large it would collapse to form a black hole

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what is a natural satellite? give an example

a satellite that is not man-made e.g the moon

<p>a satellite that is not man-made e.g the moon</p>
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are objects in orbit accelerating? explain

objects are accelerating as their direction is constantly changing which means their velocity is changing

any change in velocity is considered acceleration

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which elements undergo nuclear fusion in a main sequence star?

hydrogen nuclei fuse to make helium nuclei

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which 2 forces are in balance in a main sequence star?

outward energy pressure from heat released from nuclear fusion is balanced with inward pull of gravity

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what do we call a protostar was nuclear fusion starts?

a main sequence star

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what 2 things could a main sequence star become once it runs out of hydrogen? what determines what it becomes?

if it is relatively small, it will become a red giant

if it is relatively large, it will become a red supergiant

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are galaxies moving away from each other through space or is space itself stretching?

space & the universe itself is expanding and this makes galaxies futher apart

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for a red super giant, what happens next in the star's lifecycle?

it will explode in a supernova

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what happens when a nebula becomes very large?

gravity pulls the particles of dust and gas together to form a protostar

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how does red shift support the big bang theory?

shows that the universe is expanding as distant galaxies show a greater red shift so all galaxies are moving away from each other

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what is a neutron star?

extremely dense mass of neutrons

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what is a black hole?

a region where gravity is so strong that nothing can escape

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what must happen to an orbiting object's speed if the radius of its orbit decreases?

if the radius of the orbit decreases, the orbital speed must decrease for it to maintain a stable orbit

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what is the solar system?

consists of the sun and the objects that orbit it

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for a red giant, what happens next in the star's lifecycle?

the red giant will become a white dwarf, which will then become a black dwarf as it cools

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why does your weight vary across planets?

-your weight is dependant on g, since weight = mass x g

-the gravitational field strength (g) of a planet varies depending on the size of the planet

-this means that your weight will also vary

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which stage is the sun currently in?

main sequence

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formula for wave speed

wavelength x frequency

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blue shift

when an objects is travelling towards the earth, wavelength of the light emitted by the object decreases therefore it shifts towards the blue end of the visible light spectrum

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describe red shift

when an objects is travelling away from the earth, wavelength of the light emitted by the object increases therefore it shifts towards the red end of the visible light spectrum

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how does CMBR support the Big Bang theory?

CMBR that comes from all directions in space. it is the leftover thermal energy from the big bang

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stars can be classified in HR diagram. what do the axes of the HR diagrams represent?

x axis: decreasing temp.

y axis: absolute magnitude/luminousity

<p>x axis: decreasing temp.</p><p>y axis: absolute magnitude/luminousity</p>

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